Skip to content
DraconiticResearch
Search Sources API
197,768 studies31 sourcesUpdated 53 min ago
PreprintCC BY-NC-SA 4.0arXiv

Effects of radial conductivity variation on the Ponomarenko dynamo

Abstract

We study the effects of conductivity variation on the Ponomarenko dynamo. Taking monotonically increasing/decreasing and sinusoidally varying radial profiles, we study the kinematic dynamo problem. The threshold of the dynamo, given by the critical magnetic Reynolds number Rmc, is found to strongly depend on the form of conductivity variation near the discontinuity of the velocity field where the shear is dominant. For monotonically varying profiles in the limit of sharp variation, this threshold maps to the problem of the dynamo with a jump in conductivity, while for the sinusoidal profile with large variations/wavenumbers, the threshold increases due to effective diffusivity arising from the rapid changes in conductivity. Far from the threshold, it is found that the growth rate depends only on the local gradient of the conductivity near the discontinuity, with the opposite sign of shear and conductivity gradient leading to a larger growth rate, thereby aiding the dynamo instability in regenerating Bϕ from Br. We calculate the expression for the growth rate in the limit of large Rm(≫ 1) and find that the conductivity variation leads to a modification proportional to the local gradient of conductivity times Rm−1/2. This correction is found to depend only on the local gradient of the conductivity at the discontinuity. Similar dependencies are found for realistic, smooth velocity profiles and for different magnetic boundary conditions.

Versions

Related

  1. Can third- and fourth-order multipoles plus radial variation of iso-density ellipses explain the observed flux ratios in B1422+231? YES, and a lesson learned from a TNG100 lensing galaxy sample
    Ruizhe Feng, Dandan Xu, Dominique Sluse +3
    arXivPreprintarXiv licenceFull textCosmologyGalaxiesarXiv
  2. Exact Solution of the Direct and Inverse Quasi-stationary Dynamo Problem in the Expanding Plasma Ball
    Yurii V. Dumin
    arXivPreprintarXiv licenceFull textSolar & stellar physicsPlasma physicsarXiv
  3. The kinematic Kelvin-Helmholtz instability-driven dynamo: implications for merging compact objects
    James R. Beattie, Amitava Bhattacharjee, Elias R. Most +4
    arXivPreprintCC BY 4.0Full textGalaxiesHigh-energy astrophysicsarXiv
  4. Oscillating dynamo models with a time-nonlocal α effect
    Günther Rüdiger, Manfred Schultz, Alfio Bonanno
    arXivPreprintCC BY 4.0Full textSolar & stellar physicsarXiv
  5. Broken Power-law Distributions of Photospheric Magnetic Concentrations and Implications for Solar Dynamo
    Anchuan Song, Yuming Wang, Quanhao Zhang +2
    The Astrophysical JournalPeer-reviewedCC BY 4.0Full textSolar & stellar physicsCrossref
BibTeX
@misc{verma2026effects,
  title = {{Effects of radial conductivity variation on the Ponomarenko dynamo}},
  author = {Shipra Verma and Kannabiran Seshasayanan},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.19187},
  eprint = {2609.19187},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.19187},
  note = {CC BY-NC-SA 4.0},
}
RIS
TY  - UNPB
TI  - Effects of radial conductivity variation on the Ponomarenko dynamo
AU  - Shipra Verma
AU  - Kannabiran Seshasayanan
PY  - 2026
DA  - 2026/09/15
PB  - arXiv
DO  - 10.48550/arxiv.2609.19187
UR  - https://arxiv.org/abs/2609.19187
AB  - We study the effects of conductivity variation on the Ponomarenko dynamo. Taking monotonically increasing/decreasing and sinusoidally varying radial profiles, we study the kinematic dynamo problem. The threshold of the dynamo, given by the critical magnetic Reynolds number Rm_c, is found to strongly depend on the form of conductivity variation near the discontinuity of the velocity field where the shear is dominant. For monotonically varying profiles in the limit of sharp variation, this threshold maps to the problem of the dynamo with a jump in conductivity, while for the sinusoidal profile with large variations/wavenumbers, the threshold increases due to effective diffusivity arising from the rapid changes in conductivity. Far from the threshold, it is found that the growth rate depends only on the local gradient of the conductivity near the discontinuity, with the opposite sign of shear and conductivity gradient leading to a larger growth rate, thereby aiding the dynamo instability in regenerating B_ϕ from B_r. We calculate the expression for the growth rate in the limit of large Rm(≫ 1) and find that the conductivity variation leads to a modification proportional to the local gradient of conductivity times Rm^−1/2. This correction is found to depend only on the local gradient of the conductivity at the discontinuity. Similar dependencies are found for realistic, smooth velocity profiles and for different magnetic boundary conditions.
ER  -